activity
20052023
most citedThe CO-to-H2 Conversion Factor and Dust-to-Gas Ratio on Kiloparsec Scales in Nearby Galaxies

601 citations · 3.6k across the 47 of their papers we have counts for

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Showing 2018Show all

5 papers · 1 filter

astro-ph.GA2018★ 78 cited

WARPFIELD 2.0: Feedback-regulated minimum star formation efficiencies of giant molecular clouds

Daniel Rahner, Eric W. Pellegrini, Simon C. O. Glover +1

Star formation is an inefficient process and in general only a small fraction of the gas in a giant molecular cloud (GMC) is turned into stars. This is partly due to the negative e…

astro-ph.GA2018★ 76 cited

Feedback from massive stars at low metallicities: MUSE observations of N44 and N180 in the Large Magellanic Cloud

A. F. McLeod, J. E. Dale, C. J. Evans +5

We present MUSE integral field data of two HII region complexes in the Large Magellanic Cloud (LMC), N44 and N180. Both regions consist of a main superbubble and a number of smalle…

astro-ph.GA2018★ 38 cited

Synthetic [CII] emission maps of a simulated molecular cloud in formation

A. Franeck, S. Walch, D. Seifried +10

The C ion is an important coolant of interstellar gas, and so the [CII] fine structure line is frequently observed in the interstellar medium. However, the physical and chemi…

astro-ph.GA2018★ 30 cited

Magnetic fields in star forming systems (I): Idealized synthetic signatures of dust polarization and Zeeman splitting in filaments

Stefan Reissl, Amelia M. Stutz, Robert Brauer +3

We use the POLARIS radiative transport code to generate predictions of the two main observables directly sensitive to the magnetic field morphology and strength in filaments: dust…

astro-ph.GA2018★ 49 cited

First Results from the and ALMA Spectroscopic Surveys of the SMC: The Relationship Between [CII]-bright Gas and CO-bright Gas at Low Metallicity

Katherine E. Jameson, Alberto D. Bolatto, Mark Wolfire +15

The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present results from the Herschel S…